3-D General Relativistic MHD Simulations of Generating Jets

Details 3-D General Relativistic MHD Simulations of Generating Jets 3-D General Relativistic MHD Simulations of Generating Jets

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aas...195.6902n&link_type=abstract

American Astronomical Society, 195th AAS Meeting, #69.02; Bulletin of the American Astronomical Society, Vol. 31, p.1471

Astronomy and Astrophysics

Astronomy

1

Scientific paper

We have investigated the dynamics of an accretion disk around Schwarzschild black holes initially threaded by a uniform poloidal magnetic field in a non-rotating corona (either in a steady-state infalling state or in hydrostatic equilibrium) around a non-rotating black hole using a 3-D GRMHD with the ``axisymmetry'' along the z-direction. Magnetic field is tightly twisted by the rotation of the disk, and plasmas in the shocked region of the disk are accelerated by J x B force to form bipolar relativistic jets. In order to investigate variabilities of generated relativistic jets and magnetic field structure inside jets, we have performed calculations using the 3-D GRMHD code with a full 3-dimensional system. We will investigate how the third dimension affects the global disk dynamics and jet generation.

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